Spectral reduction package
Project description
This library was created to apply doppler tomography to the Algol star system. This is still the main purpose for most of the code.
However, some parts are generic and can be used for any spectrum and star. This includes:
flux normalization using synthetic spectra:
normalize_spectrum --help
Some example synthetic spectra from the Pollux database are included in the source distribution of the package.
planing observations of variable stars:
plan_observations --help
This scripts generates ics file you can import into your calenders.
display spectra:
fits_display1d --help
manipulate fits header:
fits_setval --help
loading spectra from fits and text files
measuring absorption or emission profiles
Attribution
There is a publication describing the flux normalization. If you publish anything using this code, please add a reference to:
@article{Brock2019, author = {Christian Brock}, title = {{C}ontinuum {N}ormalization using {S}ynthetic {S}pectra} journal = {{SPEKTRUM} Journal of the Section Spectroscopy of the Society of German Amateur Astronomers}, year = {2019}, month = {Nov}, volume= {55}, pages={4-7}, issn={2363-5894}, note={\url{{http://spektroskopie.vdsastro.de/files/pdfs/Spektrum55.pdf}} }
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